Radio signatures of solar energetic particles during the 23rd solar cycle

• DOI: 10.48550/arxiv.1402.6442
• Publication Date: 2014-01-01
• Authors: Rositsa Miteva; Karl‐Ludwig Klein; Susan W. Samwel; Alexander Nindos; Athanasios Koulou...; Hamish Reid
• Keywords: Corona (planetary geology); Solar cycle 23; Solar energetic particles; Solar flare

We present the association rates between solar energetic particles (SEPs) and radio emission signatures in corona IP space during entire cycle 23. selected SEPs associated with X M-class flares from visible hemisphere. All SEP events are also accompanied by coronal mass ejections. Here, we focus on correlation appearance of type II, III IV bursts dynamic spectra. For this used available data ground-based stations Wind/WAVES spacecraft. The associations presented separately for accompanying activity eastern western find highest rate to be bursts, followed types II IV. Whereas no longitudinal dependence is noticed, these a tendency higher SEP-association A comparison reports previous studies briefly discussed.